DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | SNR B0532-675 | 83.0766 | -67.535 | 83.105131 | -67.568522 | 336.894388 | -87.135778 | 277.71335978 | -32.44457154 | 140.0497 | 55871.6295601852 | 2011-11-06 15:06:34 | 55874.1570601852 | 2011-11-09 03:46:10 | 806007010 | 82.4909 | 80 | 82.4909 | 82.4909 | 0 | 82.4909 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 77.4573 | 77.4573 | 218.3547 | 4 | PROCESSED | 57603.7734027778 | 2016-08-03 18:33:42 | 56257 | 2012-11-26 00:00:00 | 55890.6997337963 | 2011-11-25 16:47:37 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060025 | Interstellar medium (ISM) heated by a forward shock of supernova remnants (SNRs) gives us a unique opportunity to study local metal abundance and density. Systematic study of the shock-heated ISM in a galaxy unveils its overall metal distribution and provides a key to understand its chemical evolution. On the basis of this idea, we have performed observations of SNRs in the Large Magellanic Cloud (LMC). We here propose to observe the LMC SNR B0532-675 for 80 ks. Since it locates near the star formation region LH76, we expect that we can study the process of metal diffusion from a star forming region by utilizing the result from another SNR DEM L241 near LH76 already observed. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | KENTARO SOMEYA | JAP | 6 | AO6 | STUDY OF CHEMICAL EVOLUTION OF THE LARGE MAGELLANIC CLOUD WITH SNRS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806007010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '806007010'
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